The Maxwell and Maxwell–de Rham equations can be solved exactly to first order in an external gravitational field. The gravitational background induces phases in the wave functions of spin-1 particles. These phases yield the optics of the particles without requiring any thin lens approximation.
OPTICS OF SPIN-1 PARTICLES FROM GRAVITY-INDUCED PHASES
FEOLI A;
2009-01-01
Abstract
The Maxwell and Maxwell–de Rham equations can be solved exactly to first order in an external gravitational field. The gravitational background induces phases in the wave functions of spin-1 particles. These phases yield the optics of the particles without requiring any thin lens approximation.File in questo prodotto:
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